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We study spectral densities for systems on lattices, which, at a phase transition display, power-law spatial correlations. Constructing the spatial correlation matrix we prove that its eigenvalue density shows a power law that can be…

数学物理 · 物理学 2014-11-24 Vinayak , T. Prosen , B. Buca , T. H. Seligman

We derive scaling laws for the signal-to-noise ratio of the optimal cross-correlation statistic, and show that the large power-law increase of the signal-to-noise ratio as a function of the the observation time $T$ that is usually assumed…

天体物理仪器与方法 · 物理学 2015-06-15 Xavier Siemens , Justin Ellis , Fredrick Jenet , Joseph D. Romano

The problem tackled in this paper is the determination of sample size for a given level and power in the context of a simple linear regression model. At a technical level, the simple linear regression model is a five-parameter model. It is…

统计方法学 · 统计学 2019-07-25 Tianyuan Guan , M. Khorshed Alam , M. Bhaskara Rao

We investigate the 1/f noise of the Five-hundred-meter Aperture Spherical Telescope (FAST) receiver system using drift-scan data from an intensity mapping pilot survey. All the 19 beams have 1/f fluctuations with similar structures. Both…

天体物理仪器与方法 · 物理学 2021-10-13 Wenkai Hu , Yichao Li , Yougang Wang , Fengquan Wu , Bo Zhang , Ming Zhu , Shifan Zuo , Guilaine Lagache , Yinzhe Ma , Mario G. Santos , Xuelei Chen

We present a practical implementation of a Monte Carlo method to estimate the significance of cross-correlations in unevenly sampled time series of data, whose statistical properties are modeled with a simple power-law power spectral…

天体物理仪器与方法 · 物理学 2015-06-22 W. Max-Moerbeck , J. L. Richards , T. Hovatta , V. Pavlidou , T. J. Pearson , A. C. S. Readhead

Gaussian bounds on noise correlation of functions play an important role in hardness of approximation, in quantitative social choice theory and in testing. The author (2008) obtained sharp gaussian bounds for the expected correlation of…

概率论 · 数学 2017-10-25 Elchanan Mossel

Cosmology has entered an era where the experimental limitations are not due to instrumental sensitivity but instead due to inherent systematic uncertainties in the instrumentation and data analysis methods. The field of HI intensity mapping…

宇宙学与河外天体物理 · 物理学 2018-05-23 Stuart Harper , Clive Dickinson , Richard Battye , Sambit Roychowdhury , Ian Browne , Yin-Zhe Ma , Lucas Olivari , Tianyue Chen

The three-dimensional galaxy power spectrum is a powerful probe of primordial non-Gaussianity and additional general relativistic (GR) effects on large scales, which can be constrained by the current and upcoming large-scale structure…

宇宙学与河外天体物理 · 物理学 2024-12-03 Robin Y. Wen , Henry S. Grasshorn Gebhardt , Chen Heinrich , Olivier Doré

Credit assignment--how changes in individual neurons and synapses affect a network's output--is central to learning in brains and machines. Noise correlation, which estimates gradients by correlating perturbations of activity with changes…

机器学习 · 计算机科学 2026-01-07 Byungwoo Kang , Maceo Richards , Bernardo Sabatini

We report the first detection of the ISW effect in wavelet space, at scales in the sky around 7 degrees with a significance of around 3.3 sigma, by cross-correlating the WMAP first-year data and the NRAO VLA Sky Survey (NVSS). In addition,…

天体物理学 · 物理学 2009-11-10 P. Vielva , E. Martinez-Gonzalez , M. Tucci

Despite their ability to represent highly expressive functions, deep learning models seem to find simple solutions that generalize surprisingly well. Spectral bias -- the tendency of neural networks to prioritize learning low frequency…

机器学习 · 计算机科学 2022-09-30 Sara Fridovich-Keil , Raphael Gontijo-Lopes , Rebecca Roelofs

We investigate the effect of noise on Random Boolean Networks. Noise is implemented as a probability $p$ that a node does not obey its deterministic update rule. We define two order parameters, the long-time average of the Hamming distance…

生物物理 · 物理学 2009-11-13 Tiago P. Peixoto , Barbara Drossel

The Spectral Form Factor (SFF) is a convenient tool for the characterization of eigenvalue statistics of systems with discrete spectra, and thus serves as a proxy for quantum chaoticity. This work presents an analytical calculation of the…

强关联电子 · 物理学 2022-09-07 W. L. Vleeshouwers , V. Gritsev

We present a new technique to calculate the spectral lags of gamma-ray bursts (GRBs). Unlike previous processing methods, we first smooth the light curves of gamma-ray bursts in high and low energy bands using the "Loess" filter, then, we…

高能天体物理现象 · 物理学 2015-06-04 Zhao-sheng Li , Li Chen , De-hua Wang

We report on the effect of spatially correlated noise on the velocities of self propelled particles. Correlations in the random forces acting on self propelled particles can induce directed collective motion, i.e. swarming. Even with…

软凝聚态物质 · 物理学 2022-12-21 Chunming Zheng , Ralf Tönjes

Neurons in the visual cortex are correlated in their variability. The presence of correlation impacts cortical processing because noise cannot be averaged out over many neurons. In an effort to understand the functional purpose of…

机器学习 · 计算机科学 2018-04-04 Shamak Dutta , Bryan Tripp , Graham Taylor

Presence of spectral curvature due to synchrotron self-absorption (SSA) of extragalactic radio sources may break down the spectral smoothness feature-the premise that bright radio foreground can be successfully removed in the 21cm…

宇宙学与河外天体物理 · 物理学 2015-06-05 Qian Zheng , Xiang-Ping Wu , Jun-Hua Gu , Jingying Wang , Haiguang Xu

The functional significance of correlations between action potentials of neurons is still a matter of vivid debates. In particular it is presently unclear how much synchrony is caused by afferent synchronized events and how much is…

神经元与认知 · 定量生物学 2013-04-09 Matthias Schultze-Kraft , Markus Diesmann , Sonja Grün , Moritz Helias

Spatial image quality metrics designed for camera systems generally employ the Modulation Transfer Function (MTF), the Noise Power Spectrum (NPS), and a visual contrast detection model. Prior art indicates that scene-dependent…

图像与视频处理 · 电气工程与系统科学 2019-07-23 Edward W. S. Fry , Sophie Triantaphillidou , Robin B. Jenkin , Ralph E. Jacobson , John R. Jarvis

Cosmic shear measurements rely on our ability to measure and correct the Point Spread Function (PSF) of the observations. This PSF is measured using stars in the field, which give a noisy measure at random points in the field. Using Wiener…

宇宙学与河外天体物理 · 物理学 2015-05-13 A. Amara , A. Refregier , S. Paulin-Henriksson